dc.contributor
Lompa, Tomke
dc.creator
Wünnemann, Kai
dc.identifier
https://doi.org/10.35003/BLEX70
dc.description
- We determine the size of impactors for 16 lunar far-side basins from models of isostatically compensated gravity data.</br>
- We use the elastic thickness of the lithosphere to account for isostatic relaxation of basin formation models.</br>
- Isostatic relaxation of lunar farside basins depends on impactor size and formation time and affects the gravity signature of basins.
dc.subject
Astronomy and Astrophysics
dc.subject
Computer and Information Science
dc.subject
Impact Processes
dc.title
Replication Data for: Evolution of Impact Basin Gravity Signatures on the Lunar Farside: A long-term Alteration Process